Results of CRESST phase I
Results of the CRESST experiment at Gran Sasso using 262 g sapphire calorimeters with tungsten phase transition thermometers are presented. Calibration and analysis methods are described. Data taken in 2000 have been used to place limits on WIMP dark matter particles in the galactic halo. The sapphi...
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| Formáid: | Conference item |
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2002
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| _version_ | 1826282398392778752 |
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| author | Probst, F Angloher, G Bruckmayer, M Bucci, C Cooper, S Di Stefano, P von Feilitzsch, F Frank, T Hauff, D Jagemann, T Jochum, J Keeling, R Kraus, H Marchese, J Ramachers, Y Schnagl, J Seidel, W Sergeyev, I Stark, M Stodolsky, L Wulandari, H |
| author_facet | Probst, F Angloher, G Bruckmayer, M Bucci, C Cooper, S Di Stefano, P von Feilitzsch, F Frank, T Hauff, D Jagemann, T Jochum, J Keeling, R Kraus, H Marchese, J Ramachers, Y Schnagl, J Seidel, W Sergeyev, I Stark, M Stodolsky, L Wulandari, H |
| author_sort | Probst, F |
| collection | OXFORD |
| description | Results of the CRESST experiment at Gran Sasso using 262 g sapphire calorimeters with tungsten phase transition thermometers are presented. Calibration and analysis methods are described. Data taken in 2000 have been used to place limits on WIMP dark matter particles in the galactic halo. The sapphire detectors are especially sensitive for low-mass WIMPS with spin-dependent interaction and improve on existing limits in this region. |
| first_indexed | 2024-03-07T00:43:15Z |
| format | Conference item |
| id | oxford-uuid:83c77b2e-bf3d-4ef9-b6c0-cf0bf8d2db87 |
| institution | University of Oxford |
| last_indexed | 2024-03-07T00:43:15Z |
| publishDate | 2002 |
| record_format | dspace |
| spelling | oxford-uuid:83c77b2e-bf3d-4ef9-b6c0-cf0bf8d2db872022-03-26T21:46:30ZResults of CRESST phase IConference itemhttp://purl.org/coar/resource_type/c_5794uuid:83c77b2e-bf3d-4ef9-b6c0-cf0bf8d2db87Symplectic Elements at Oxford2002Probst, FAngloher, GBruckmayer, MBucci, CCooper, SDi Stefano, Pvon Feilitzsch, FFrank, THauff, DJagemann, TJochum, JKeeling, RKraus, HMarchese, JRamachers, YSchnagl, JSeidel, WSergeyev, IStark, MStodolsky, LWulandari, HResults of the CRESST experiment at Gran Sasso using 262 g sapphire calorimeters with tungsten phase transition thermometers are presented. Calibration and analysis methods are described. Data taken in 2000 have been used to place limits on WIMP dark matter particles in the galactic halo. The sapphire detectors are especially sensitive for low-mass WIMPS with spin-dependent interaction and improve on existing limits in this region. |
| spellingShingle | Probst, F Angloher, G Bruckmayer, M Bucci, C Cooper, S Di Stefano, P von Feilitzsch, F Frank, T Hauff, D Jagemann, T Jochum, J Keeling, R Kraus, H Marchese, J Ramachers, Y Schnagl, J Seidel, W Sergeyev, I Stark, M Stodolsky, L Wulandari, H Results of CRESST phase I |
| title | Results of CRESST phase I |
| title_full | Results of CRESST phase I |
| title_fullStr | Results of CRESST phase I |
| title_full_unstemmed | Results of CRESST phase I |
| title_short | Results of CRESST phase I |
| title_sort | results of cresst phase i |
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